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<ri:Resource created="2026-05-07T10:38:19Z" status="active" updated="2026-05-07T13:53:31Z" version="1.2" xmlns:cs="http://www.ivoa.net/xml/ConeSearch/v1.0" xmlns:ri="http://www.ivoa.net/xml/RegistryInterface/v1.0" xmlns:vr="http://www.ivoa.net/xml/VOResource/v1.0" xmlns:vs="http://www.ivoa.net/xml/VODataService/v1.1" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.ivoa.net/xml/ConeSearch/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/ConeSearch.xsd http://www.ivoa.net/xml/VOResource/v1.0 http://vo.ari.uni-heidelberg.de/docs/schemata/VOResource.xsd http://www.ivoa.net/xml/VODataService/v1.1 http://vo.ari.uni-heidelberg.de/docs/schemata/VODataService.xsd" xsi:type="vs:CatalogService"><title>Milky Way as seen by classical Cepheids. I. WISE</title><shortName>J/ApJS/278/57</shortName><identifier>ivo://CDS.VizieR/J/ApJS/278/57</identifier><curation><publisher ivo-id="ivo://CDS">CDS</publisher><creator><name>Skowron D.M.</name></creator><creator><name>Drimmel R.</name></creator><creator><name>Khanna S.</name></creator><creator><name>Spagna A.</name></creator><creator><name>Poggio E.</name></creator><creator><name>Ramos P.</name></creator><date role="Updated">2026-05-07T13:53:31Z</date><date role="Created">2026-05-07T10:38:19Z</date><contact><name>CDS support team</name><address>CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France</address><email>cds-question@unistra.fr</email></contact></curation><content><subject>variable-stars</subject><subject>infrared-photometry</subject><subject>stellar-distance</subject><subject>extinction</subject><subject>stellar-ages</subject><subject>visible-astronomy</subject><subject>milky-way-galaxy</subject><description>Classical Cepheids are the archetype of the standard candle, thanks to the period-luminosity relation, which allows us to measure their intrinsic brightness. They are also relatively young and bright, potentially making them excellent tracers of the young stellar population that is responsible for shaping the visible aspect of our Galaxy. However, being observers embedded in the dusty interstellar medium of the Galaxy, deriving reliable photometric distances to classical Cepheids of the Milky Way is a challenge. The typical approach is to use "reddening-free" indices, such as Wesenheit magnitudes, to obviate the need for an extinction correction. However, this approach could lead to unknown systematics-especially toward the inner Galaxy-as its assumption of a universal total-to-selective extinction ratio is not satisfied, particularly in lines of sight where the extinction is high and crosses spiral arms. We instead estimate new distances for 3424 Cepheids based on mid-IR photometry from the Wide-field Infrared Survey Explorer, which suffers minimally from extinction, and by adopting a 3D extinction map to calculate the necessary (albeit small) extinction corrections. We show that our distances are consistent with Gaia's parallaxes for the subset with relative parallax errors smaller than 10%, verifying that our mean distance errors are of the order of 6% and that the mean parallax zero-point for this subsample is 7{mu}as.</description><source format="bibcode">2025ApJS..278...57S</source><referenceURL>https://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/278/57</referenceURL><type>Catalog</type><contentLevel>Research</contentLevel><relationship><relationshipType>IsServedBy</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/TAP">TAP VizieR generic service</relatedResource></relationship><relationship><relationshipType>IsServedBy</relationshipType><relatedResource>Conesearch service</relatedResource></relationship><relationship><relationshipType>related-to</relationshipType><relatedResource ivo-id="ivo://CDS.VizieR/B/gcvs">B/gcvs : General Catalogue of Variable Stars (Samus+, 2007-2017)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/B/corot">B/corot : CoRoT observation log (N2-4.4) (CoRoT 2016)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/273">II/273 : MISAO new variable stars (Yoshida+, 1999-2000)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/264">II/264 : ASAS Variable Stars in Southern hemisphere (Pojmanski+, 2002-2005)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/287">II/287 : Northern Sky Variability Survey (NSVS) (Wozniak+, 2004)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/311">II/311 : WISE All-Sky Data Release (Cutri+ 2012)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/328">II/328 : AllWISE Data Release (Cutri+ 2013)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/I/345">I/345 : Gaia DR2 (Gaia Collaboration, 2018)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/363">II/363 : The band-merged unWISE Catalog (Schlafly+, 2019)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/366">II/366 : ASAS-SN catalog of variable stars (Jayasinghe+, 2018-2020)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/II/365">II/365 : The CatWISE2020 catalog (updated version 28-Jan-2021) (Marocco+, 2021)</relatedResource><relatedResource ivo-id="ivo://CDS.VizieR/V/155">V/155 : GDR2AP. 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The format may include more digits than the original data because of internal accuracy requirements in VizieR and across other CDS services)</description><unit>deg</unit><ucd>pos.eq.dec</ucd><flag>indexed</flag></column><column><name>e_muAll</name><description>[0/0.6] Uncertainty in muAll (e_mu_all)</description><unit>mag</unit><ucd>stat.error;phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Period</name><description>[0.26/68.7] Fundamentalized period of variability from P21 (Pietrukowicz+ 2021AcA....71..205P) (period)</description><unit>d</unit><ucd>time.period</ucd><dataType xsi:type="vs:VOTableType">double</dataType></column><column><name>W1magAll</name><description>[0/15.1] Apparent W1 magnitude from AllWISE after corrections (w1_all)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um;arith.diff</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>muAll</name><description>[0/20] Distance modulus based on AllWISE (mu_all)</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DistAll</name><description>[0/98815] Distance based on AllWISE (d-all)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_DistAll</name><description>[0/4429] Uncertainty in DistAll (d-all)</description><unit>pc</unit><ucd>stat.error;pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Aw1All</name><description>[0/1.1] Extinction in W1 from AllWISE (a_all)</description><unit>mag</unit><ucd>phys.absorption;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W1magUn</name><description>[0/15.6] Apparent W1 magnitude from unWISE (w1_un)</description><unit>mag</unit><ucd>phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>muUn</name><description>[0/21.3] Distance modulus based on unWISE (mu_un)</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_muUn</name><description>[0/0.12] Uncertainty in muUn (e_mu_un)</description><unit>mag</unit><ucd>stat.error;phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>DistUn</name><description>[0/180882] Distance based on unWISE (d_un)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_DistUn</name><description>[0/7147] Uncertainty in DistUn (e_d_un)</description><unit>pc</unit><ucd>stat.error;pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Aw1Un</name><description>[0/1.21] Extinction in W1 from unWISE (a_un)</description><unit>mag</unit><ucd>phys.absorption;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>W1mag</name><description>[0.3/15.6] Apparent W1 magnitude averaged over AllWISE and unWISE (w1_av)</description><unit>mag</unit><ucd>stat.mean;phot.mag;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>mu</name><description>[5.67/21.3] Distance modulus based on averaged W1 (mu_av)</description><unit>mag</unit><ucd>phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>e_mu</name><description>[0.08/0.6] Uncertainty in mu (e_mu_av)</description><unit>mag</unit><ucd>stat.error;phot.mag.distMod</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Dist</name><description>[136/180882] Distance based on averaged W1 (d_av)</description><unit>pc</unit><ucd>pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>e_Dist</name><description>[6/7147] Uncertainty in Dist (e_d_av)</description><unit>pc</unit><ucd>stat.error;pos.distance</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Aw1</name><description>[0/1.21] Extinction in W1 based on averaged W1 (a_av)</description><unit>mag</unit><ucd>phys.absorption;em.IR.3-4um</ucd><dataType xsi:type="vs:VOTableType">float</dataType></column><column><name>Age</name><description>[14/1243] Age estimate (age)</description><unit>Myr</unit><ucd>time.age</ucd><dataType xsi:type="vs:VOTableType">int</dataType></column><column><name>Q</name><description>[0/42.6]? Quality indicator</description><ucd>meta.code.qual</ucd><dataType xsi:type="vs:VOTableType">double</dataType><flag>nullable</flag></column><column><name>S19</name><description>Display data from Skowron+ 2019, J/AcA/69/305 within 3"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType">int</dataType><flag>nullable</flag></column><column><name>WISEA</name><description>Display data from AllWISE (II/328) within 1"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column><column><name>unWISE</name><description>Display data from unWISE (II/363) within 1"</description><ucd>meta.ref.url</ucd><dataType xsi:type="vs:VOTableType" arraysize="*">char</dataType></column></table></schema></tableset></ri:Resource>